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This is an old revision of this page, as edited by Zandperl (talk | contribs) at 15:23, 16 February 2004 (wikiproject telescopes?). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

I have remove the following statement, which I think correspond not to spherical aberration but field curvature. -- looxix 19:33 Apr 21, 2003 (UTC)

Some schmidt cassegrains have intentional spherical aberration, and compensate with a film-holder that stretches the film into a mild spherical shape.

The Telescope mountings para is largely incomplete lacks equatorial and meridian mount. Ericd 01:47 Apr 22, 2003 (UTC)

I am not conviced by :

"The phenomenon of optical diffraction sets a limit to the resolution and image quality that any telescope can achieve. We still do not know when this limit will be reached, but most astronomers believe we will reach it sooner or later."

IMO diffraction occurs with a small apertures and research telescope have large apertures.

But, I'm not a specialist. Ericd 17:56, 2 Oct 2003 (UTC)

You can read about the influence of diffraction on resolution limits at the [link provided at the bottom of the page, but I'll clarify in the article. Nixdorf 23:08, 3 Oct 2003 (UTC)

Would anyone be interested helping with a Wikipedia:WikiProject Telescopes and/or Wikipedia:WikiProject Space Telescopes? Should a telescopes template include space telescopes? It/they could be modeled after the following articles:

--zandperl 15:23, 16 Feb 2004 (UTC)